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1514 Ricouxa
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Asteroid of the inner regions of the asteroid belt
October 2019
yes
1514 Ricouxa
#D6D6D6
001514-asteroid shape model (1514) Ricouxa.png
Shape model of Ricouxa from its lightcurve
22 August 1906
M. F. Wolf
Heidelberg Obs.
(1514) Ricouxa
1906 UR1936 ME1939 HC1940 XA1970 XAA916 OC
unknown(named by A. Patry)
main-beltFlora
4 September 2017 (JD 2458000.5)
0
110.06 yr (40,198 days)
2.6876 AU
1.7937 AU
2.2407 AU
0.1995
3.35 yr (1,225 days)
41.914°
0.2939 ms / day
4.5349°
145.85°
179.38°
6.66 0.27 km7.07 km (derived)7.784 0.062 km8.129 0.021 km
10.033 0.002 h10.42466 h10.42468 0.00005 h10.438 h
0.1821 0.03970.228 0.0390.24 (assumed)0.363 0.046
S
12.6012.79 0.1712.812.92
1514 Ricouxa (provisional designation 1906 UR) is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7.5 kilometers in diameter. It was discovered on 22 August 1906, by German astronomer Max Wolf at Heidelberg Observatory in southern Germany. The origin of the asteroid's name is unknown.
Classification and orbit
Ricouxa is a S-type asteroid and member of the Flora family, one of the largest collisional populations of stony asteroids in the entire main-belt. It orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,225 days). Its orbit has an eccentricity of 0.20 and an inclination of 5° with respect to the ecliptic. Ricouxa's observation arc begins with its official discovery observation in 1906, as no precoveries were taken, and no prior identifications were made.
Physical characteristics
Rotation and poles
In the 1990s, Italian astronomer Maria A. Barucci obtained a rotational lightcurve of Ricouxa, using the ESO 1-metre telescope at La Silla Observatory in Chile. Lightcurve analysis gave a well-defined rotation period of 10.438 hours with a brightness variation of 0.62 magnitude (U=3).
Photometric observations by French amateur astronomer Pierre Antonini in April 2006, gave a similar period of 10.033 hours and an identical amplitude of 0.62 magnitude (U=2+). Additional periods were derived on modeled light-curves from various data sources. They gave a period of 10.42466 and 10.42468 hours, as well as a spin axis of (0°, 71.0°) and (251.0°, 75.0°) in ecliptic coordinates, respectively.
Diameter and albedo
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Ricouxa measures 7.78 kilometers in diameter, and its surface has an albedo of 0.228 (revised albedo-fits per 2014), while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – taken from 8 Flora, the family's principal body and namesake – and derives a diameter of 7.07 kilometers based on an absolute magnitude of 12.92.
Naming
This minor planet was named by French astronomer André Patry (1902–1960), after whom the asteroid 1601 Patry is named. However, any reference to a person or occurrence for the name "Ricouxa" remains unknown. The asteroid's name was also published in The Names of the Minor Planets by Paul Herget in 1955 (H 135).
Unknown meaning
Among the many thousands of named minor planets, Ricouxa is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 164 Eva and 1514 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.
References
2016-09-11 last obs.
JPL Small-Body Database Browser: 1514 Ricouxa (1906 UR)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001514
Jet Propulsion Laboratory
5 June 2017
Dictionary of Minor Planet Names – (1514) Ricouxa
Schmadel Lutz D.
Springer Berlin Heidelberg
120
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1515 (1514) Ricouxa
Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision
Appendix 11 – Minor Planet Names with Unknown Meaning
Schmadel Lutz D.
Springer Berlin Heidelberg
927–929
2007
978-3-540-00238-3
Lutz D. Schmadel
1514 Ricouxa (1906 UR)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1514
4 January 2017
Asteroids and comets rotation curves – (1514) Ricouxa
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001514
4 January 2017
3 August 2003
https://web.archive.org/web/20030803183423/http://obswww.unige.ch/~behrend/page4cou.html#001514
dead
6
Joseph R. Masiero
T. Grav
A. K. Mainzer
C. R. Nugent
J. M. Bauer
R. Stevenson
S. Sonnett
August 2014
Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
4 January 2017
1514
4 January 2017
6
A. Mainzer
T. Grav
J. Masiero
E. Hand
J. Bauer
D. Tholen
R. S. McMillan
T. Spahr
R. M. Cutri
E. Wright
J. Watkins
W. Mo
C. Maleszewski
November 2011
NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
C. Nugent
M. S. Cabrera
November 2012
Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
The Astrophysical Journal Letters
759
1
5
2012ApJ...759L...8M
10.1088/2041-8205/759/1/L8
1209.5794
4 January 2017
M. A. Barucci
M. di Martino
E. Dotto
M. Fulchignoni
A. Rotundi
R. Burchi
June 1994
Rotational properties of small asteroids: Photoelectric observations of 16 asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1994Icar..109..267B
Icarus
109
2
267–273
0019-1035
1994Icar..109..267B
10.1006/icar.1994.1092
4 January 2017
6
J. Durech
M. Kaasalainen
B. D. Warner
M. Fauerbach
S. A. Marks
S. Fauvaud
M. Fauvaud
J.-M. Vugnon
F. Pilcher
L. Bernasconi
R. Behrend
January 2009
Asteroid models from combined sparse and dense photometric data
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009A&A...493..291D
Astronomy and Astrophysics
493
1
291–297
2009A&A...493..291D
10.1051/0004-6361:200810393
4 January 2017 free
6
Hanus, J.
Durech, J.
Broz, M.
Warner, B. D.
Pilcher, F.
Stephens, R.
Oey, J.
Bernasconi, L.
Casulli, S.
Behrend, R.
Polishook, D.
Henych, T.
Lehký, M.
Yoshida, F.
Ito, T.
June 2011
A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011A&A...530A.134H
Astronomy & Astrophysics
530
16
2011A&A...530A.134H
10.1051/0004-6361/201116738
1104.4114
4 January 2017
6
Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
William S. Burgett
Kenneth C. Chambers
Heather Flewelling
Nick Kaiser
Eugen A. Magnier
Jeff S. Morgan
Paul A. Price
John L. Tonry
Christopher Waters
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External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1514
1513 Mátra 1514 1515 Perrotin
001514
Category:Discoveries by Max Wolf
Category:Named minor planets
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